... 1995: . ... for the first time a magnetic field was registered on normal white dwarfs. ... A study of variability of the first galactic superluminal radio source GRO J1915 +10 with the RATAN-600 showed a delay of flare activity at 3 frequencies of 5-10 days after the X-ray flares with an inversion of the radio spectrum. ... The distribution of linear dimensions of clouds in the first approximation is power-law. The distribution of clouds by concentrations depends on the galactic latitude. ...

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... We address a question if globular clusters (GC) in a protogalaxy could for some time evolve chemically as isolated systems, enriching themselves with heavy elements produced in first supernova events that follow initial star formation. We determine both the critical mass of a protoglobular cluster that is needed to retain the ejecta of the very first supernova, and the critical energy (i.e., number of supernovae) that is needed to expel the residual gas from a cluster of a given mass. ...

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The compression of the cloud of gas in star forming . ... These data have allowed us to create the dynamic model of the cloud of gas, around this object. ... The results on H2CO absorption lines (figure 1) have shown, that the central part of the cloud represents a clumped envelope of diameter 9 pc with radial velocity 20 km/s. The relation of radial velosity of absorption line and the whole object have allowed simple to define the direction of radial movement - itis compression. ...

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• Experiment COLD: Astrophysical Problems Studied in Experiment Cold
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On the inclination of planetary orbits! Caroline Terquem! ... Planets on inclined orbits Higher inclinations for planets around stars with Teff>6250K? Planet formation, Hot Jupiters and misalignments 1. If planets form by the core accretion scenario and migrate in: Hot Jupiters But no eccentricity and no misalignment (if the disc is in the star's equatorial plane) With further planet/planet scattering and/or Kozai cycles: Eccentricity and misalignment But companions required.. ...

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• http://www.mrao.cam.ac.uk/~krause/mk.windjet.small.pdf

... 2009) 0 Fig.1 Ї Max-Planck-Institute for Radioastronomy, Bonn , VLBI ESO, COMPONENTS PARAMETERS FROM INTERFEROMETRY Ї Following S.Kraus et al. ... Using i=105o , we obtain v sini = 32 km/s. BEST MODEL FIT 1OriC 1 Ї Mass, M Ї Luminosity, log L Ї Radius, R Ї Teff, K Ї log g Ї Equatorial rotation velocity, km/s Ї Magnetic field , G Ї The time of life, yrs 35.8 5.20 10.0 37000 4.01 5.4 500-1500 150 000 1OriC 2 10.0 4.69 8.2 30000 3.60 96.2 moves to MS 1 OriC ...

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... Journal of the Amateur Astronomers Association of New York December 2015 V olume 64 Number 12; ISSN 0146-7662 Our Solo Sun Stranded without Star Siblings AAA LECTURE SERIES By Rafael Ferreira Double-sun planets like Tatooine from Star Wars are no longer the stuff of science fiction ґ thanks to Kepler. ... Yes, the gravity that you experience on Earth every day is the key component to making stars. ... Disk fragmentation usually occurs for stars with 10 or more solar masses. ...

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Where Some Asteroid Parent Bodies V. V. Busarev, Sternberg State Astronomical Institute, Moscow University, Moscow, Russian Federation; e-mail: busarev@sai.msu.ru Summary: From analysis of observational data and results of contemporary cosmogonic models a hypothesis is propounded on intensive production of dust in the asteroid belt during a postaccretionary period. ... In this process a large number of asteroid parent bodies or fragments were probably swept out of the asteroid belt [17, 24]. ...

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• http://selena.sai.msu.ru/Bus/Publications/EM&P2003(Bus-Dor-Mak).pdf
• http://selena.sai.msu.ru/Bus/Publications/SSR-05(Prok-Boch-Bus).pdf
• http://selena.sai.msu.ru/Ber/Publications/ilewg4.pdf

... Sunrise Registration of participants Opening of the conference and Memorial Coffee break Plenary session Lunch Section session Coffee break Section sessions Dinner Guitar concert in memory of A.Shevchenko. ... Section Planetarium of Ukraine 14.30 ґ18.00 Conference Room (2 floor) 5-th Gamow International Conference in Odessa Astrophysics and Cosmology after Gamow: progress and perspectives and 15-th Gamow Summer School Astronomy ... Shtanov Yu.V. PURE-CONNECTION THEORY OF GRAVITY (20 min)...

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• http://www.astro-soc.odessa.ua/Public-2010.pdf

... 319, P 365-370 (1997). ... Article in PDF format (403 KB) . ... 319, P 371-374 (1997). ... 319, P 375-393 (1997). ... 319, P 394-396 (1997). ... 319, P 397-400 (1997). ... 319, P 401-404 (1997). ... 319, P 405-412 (1997). ... 319, P 413-429 (1997). ... 319, P 430-434 (1997). ... 319, P 435-449 (1997). ... 319, P 450-458 (1997). ... 319, P 459-469 (1997). ... 319, P 470-480 (1997). ... 319, P 481-486 (1997). ... 319, P 487-497 (1997). ... 319, P 498-506 (1997). ... helpdesk@link.springer.de . ...

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• Springer LINK:A&A-EE: Table of Contents Volume 328 Number 2 (1997)
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Stanislav Shalunov How can an internet work and how does the Internet work MCCME Moscow, 1998 2 Contents 1 Introduction 1.1 How to read this book . . . . . . . . . . . . . . . . . . . . 1.2 Why and where to get the RFCs . . . . . . . . . . . . . . 1.3 Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . 6 6 7 8 2 Thin Ethernet as an example of the physical layer 3 Internet Protocol (IP) 2.1 Media Access Control (MAC) addresses . . . . . . . . . . 10 2.2 Collisions . . . . . . . . . . . . . . . . .

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• http://www.mccme.ru/computers/inetwork.ps

... The fireball flew on February 15, 2013 at 09:22 (03:22 UTC) in Chelyabinsk region at supersonic speed and with bright flashes of light along the trajectory of the NEE-SWW( Chelyabinsk-Miass-Satka ). ... On March 21, 2013 at 14:00 Sternberg Astronomical Institute (SAI MSU) held joint seminar organized INASAN, IDG, Vernadsky Institute, IKI RAS and SAI MSU for the results of meteorite Chelyabinsk study. ... Russian scientists of Vernadsky Institute analyse Chebarkul/Chelyabinsk Meteorite ( Vesti.Ru ) ....

32. Multi-threaded Query Agent and Engine for a Very Large Astronomical Database